Gulliver 55
0.78
UTI
0.5
CN
0.91
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
3.9 [arcmin]
- CN 0.5 Moderately populated
- Cdens 0.91 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Gulliver 55 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Relatively close
Low extinction
Near-solar metallicity
Old
Contains BSS
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 297.83 | 18.664 | 0.343 | -2.026 | -2.542 | 24.421 |
| Li et al. | 2025 | 297.833 | 18.661 | 0.369 | -2.043 | -2.53 | â |
| Hu & Soubiran | 2025 | 297.828 | 18.662 | â | â | â | â |
| Almeida et al. | 2025 | 297.832 | 18.65 | â | â | â | â |
| Hunt & Reffert | 2024 | 297.83 | 18.675 | 0.346 | -2.061 | -2.597 | 24.816 |
| Cavallo et al. | 2024 | 297.828 | 18.662 | 0.348 | â | â | â |
| Hunt & Reffert | 2023 | 297.83 | 18.675 | 0.346 | -2.061 | -2.597 | 24.816 |
| Rain et al. | 2021 | 297.833 | 18.661 | 0.369 | -2.043 | -2.53 | â |
| Dias et al. | 2021 | 297.832 | 18.65 | 0.368 | -2.062 | -2.52 | 24.333 |
| Cantat-Gaudin et al. | 2020 | 297.833 | 18.661 | 0.369 | -2.043 | -2.53 | â |
| Cantat-Gaudin & Anders | 2020 | 297.833 | 18.661 | 0.369 | -2.043 | -2.53 | â |
| Monteiro & Dias | 2019 | 297.833 | 18.661 | â | â | â | 2.385 |
| Soubiran et al. | 2018 | 297.833 | 18.661 | â | â | â | 24.21 |
| Cantat-Gaudin et al. | 2018 | 297.833 | 18.661 | 0.369 | -2.043 | -2.53 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.40 | 1.29 | â | 1979 | -0.364 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.130* | â | â | â |
| Almeida et al. | 2025 | 2.52 | 0.86 | â | 2382 | â | 74 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 373* | â | â |
| Cavallo et al. | 2024 | 2.37 | 1.05 | â | 741 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 2.65 | 1.16 | 1.24 | 571 | â | â | â | â |
| Rain et al. | 2021 | 2.51 | 0.87 | â | 1585 | â | â | â | 3 |
| Dias et al. | 2021 | 2.52 | 0.86 | â | 2382 | 0.112 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.37 | 0.92 | â | 1995 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.51 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 2.34 | 0.88 | â | 1614 | 0.048 | â | â | â |
| Soubiran et al. | 2018 | 2.51 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.51 | â | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.